Мир вокруг нас
Шрифт:
61. Franz Muheim (2006). "Junior Honours Nuclear and Particle Physics — Part II: Particle Physics". The University of Edinburgh. Lecture 10, p. 3. http://www2.ph.ed.ac.uk/~muheim/teaching/np3/lect-ZandW.pdf
62. Ишханов Б.С., Кэбин Э.И. «Шпаргалка для отличника (Частицы и ядра) — Глюоны». МГУ. http://nuclphys.sinp.msu.ru/spargalka/053.htm
63. M.A. Thomson (Lent 2004). "Lecture Courses — Part II, Particle Physics — QCD". University of Cambridge. P. 4. http://www.hep.phy.cam.ac.uk/~thomson/lectures/partIIparticles/pp2004_qcd.pdf
64. Ишханов Б.С., Кэбин Э.И. «Антиматерия». МГУ. Гл. 11. http://nuclphys.sinp.msu.ru/antimatter/ant11.htm
65. "CNO cycle". Wikipedia. Web. 29 ноя. 2014. http://en.wikipedia.org/wiki/CNO_cycle
66. Надежин Д.К. «Углеродный цикл». Физика Космоса — Маленькая Энциклопедия / Гл. ред. Р. А. Сюняев, 2-е изд. — М.: Советская Энциклопедия, 1986.
67. F. Palla, H. Zinnecker (2002). A. Maeder, G. Meynet, eds. "Physics of Star Formation in Galaxies". Springer, рp. 25, 43.
68. Fred C. Adams (1996). Ben Zuckerman, Matthew A. Malkan, eds. "The Origin and Evolution of the Universe". Jones & Bartlett, pp. 46–47.
69. F. Palla, H. Zinnecker (2002). A. Maeder, G. Meynet, eds. "Physics of Star Formation in Galaxies". Springer, рp. 43, 45.
70. "Red dwarf star". Encyclopaedia Britannica. Web. 30 ноя. 2014. http://www.britannica.com/EBchecked/topic/494217/red-dwarf-star
71. Philip Massey, Michael R. Meyer (October 2001). "Stellar Masses". Encyclopedia of Astronomy and Astrophysics. Nature Publishing Group and Institute of Physics Publishing, pp. 1–3. http://www.astro.caltech.edu/~george/ay20/eaa-stellarmasses.pdf
72. Fred C. Adams, Gregory Laughlin, and Genevieve J. M. Graves (2004). "Red Dwarfs and the End of the Main Sequence". RevMexAA (Serie de Conferencias), 22, 46–49, p. 47. http://www.astroscu.unam.mx/rmaa/RMxAC..22/PDF/RMxAC..22_adams.pdf
73. Peter P. Eggleton, John Faulkner (1981). I. Iben Jr. and A. Renzini (eds.). "Why Do Stars Become Red Giants?". Physical Processes in Red Giants, 179–182. Springer, pp. 179–180. DOI: http://dx.doi.org/10.1007/978-94-009-8492-9_18
74. O.R. Pols (September 2011). "Stellar Structure and Evolution". Astronomical Institute Utrecht. P. 150. Web. 2 дек. 2014. http://www.ucolick.org/~woosley/ay112-14/texts/pols11.pdf
75. "Triple-alpha process". Wikipedia. Web. 4 дек. 2014. http://en.wikipedia.org/wiki/Triple-alpha_process
76. Kragh, Helge (07 Oct 2010). "When is a prediction anthropic? Fred Hoyle and the 7.65 MeV carbon resonance". University of Aarhus. P. 18. http://philsci-archive.pitt.edu/5332/
77. C.R. Nave. "The Hoyle Resonance". HyperPhysics. Georgia State University. Web. 4 дек. 2014. http://hyperphysics.phy-astr.gsu.edu/hbase/astro/helfus.html#c2
78. Ишханов Б.C., Капитонов И.М., Тутынь И.А. «Нуклеосинтез во Вселенной». — М.: Изд-во Московского университета, 1998. — Гл. 6. http://nuclphys.sinp.msu.ru/nuclsynt/n06.htm
79. L. Siess (December III 2007). "Evolution of massive AGB stars — II. model properties at non-solar metallicity and the fate of Super-AGB stars". A &A 476 (2), 893–909, pp. 895–896, 898. DOI: http://dx.doi.org/10.1051/0004-6361:20078132
80. Sean G. Ryan, Andrew J. Norton (2010). "Stellar Evolution and Nucleosynthesis". Cambridge University Press, p. 109.
81. Albert A. Zijlstra (7 Nov 1994). "Stellar Evolution and Mass Loss on the Asymptotic Giant Branch", p. 1. arXiv: http://arxiv.org/abs/astro-ph/9411023v1
82. Daniel J. Eisenstein et al. (2006 November). "A Catalog of Spectroscopically Confirmed White Dwarfs from the Sloan Digital Sky Survey Data Release 4". The Astrophysical Journal Supplement Series, 167 40–58, p. 40. DOI: http://dx.doi.org/10.1086/507110
83. Mukremin Kilic et al. (2007 May 10). "The Lowest Mass White Dwarf". The Astrophysical Journal, 660 1451–1461, p. 1460. DOI: http://dx.doi.org/10.1086/514327
84. S. O. Kepler et al. (March 11, 2007). "White dwarf mass distribution in the SDSS". Mon. Not. R. Astron. Soc. 375, 1315–1324, p. 1315. DOI: http://dx.doi.org/10.1111/j.1365-2966.2006.11388.x
85. Ишханов Б.C., Капитонов И.М., Тутынь И.А. «Нуклеосинтез во Вселенной — Белый карлик». — М.: Изд-во Московского университета, 1998. http://nuclphys.sinp.msu.ru/nuclsynt/n10a.htm
86. Shipman, H. L. (Feb. 15, 1979). "Masses and radii of white-dwarf stars. III — Results for 110 hydrogen-rich and 28 helium-rich stars". The Astrophysical Journal, 228, 240–256, p. 255. http://adsabs.harvard.edu/abs/1979ApJ...228..240S
87. P.-E. Tremblay and P. Bergeron (2008 January 10). "The Ratio of Helium — to Hydrogen-Atmosphere White Dwarfs: Direct Evidence for Convective Mixing". The Astrophysical Journal, 672 1144–1152, p. 1144. DOI: http://dx.doi.org/10.1086/524134
88. L. Siess (March III 2006). "Evolution of massive AGB stars — I. Carbon burning phase". Astronomy and Astrophysics 448 (2), 717–729, pp. 724–725. DOI: http://dx.doi.org/10.1051/0004-6361:20053043
89. Carlos A. Bertulani (2007). "Nuclear Physics in a Nutshell". Princeton University Press, pp. 363–364.
90. L. Siess (December III 2007). "Evolution of massive AGB stars — II. model properties at non-solar metallicity and the fate of Super-AGB stars". A &A 476 (2), 893–909, pp. 895–896. DOI: http://dx.doi.org/10.1051/0004-6361:20078132
91. C. de Loore, C. Doom (1992). Edited by C. de Loore. "Structure and Evolution of Single and Binary Stars". Springer, p. 95.
92. L. Siess (December III 2007). "Evolution of massive AGB stars — II. model properties at non-solar metallicity and the fate of Super-AGB stars". A &A 476 (2), 893–909, p. 899. DOI: http://dx.doi.org/10.1051/0004-6361:20078132
93. Marco Limongi, Oscar Straniero, and Alessandro Chieffi (2000 August). "Massive Stars in the Range 13–25 M